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Identification of red high proper-motion objects in Tycho-2 and 2MASS catalogues using Virtual Observatory tools

机译:使用虚拟天文台工具识别Tycho-2和2MASS目录中的红色高准运动物体

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Aims. With available Virtual Observatory tools, we looked for new M dwarfs in the solar neighbourhood and M giants with high tangential velocities. Methods. From an all-sky cross-match between the optical Tycho-2 and the near-infrared 2MASS catalogues, we selected objects with proper motions μ??>??50?mas?yr-1 and very red VT???Ks colours. For the most interesting targets, we collected multi-wavelength photometry, constructed spectral energy distributions, estimated effective temperatures and surface gravities from fits to atmospheric models, performed time-series analysis of ASAS V-band light curves, and assigned spectral types from low-resolution spectroscopy obtained with CAFOS at the 2.2?m Calar Alto telescope. Results. We got a sample of 59 bright red high proper-motion objects, including fifty red giants, four red dwarfs, and five objects reported in this work for the first time. The five new stars have magnitudes VT??≈??10.8–11.3?mag, reduced proper motions midway between known dwarfs and giants, near-infrared colours typical of giants, and effective temperatures Teff??≈??2900–3400?K. From our time-series analysis, we discovered a long secondary period in Ruber?4 and an extremely long primary period in Ruber?6. With the CAFOS spectra, we confirmed the red giant nature of Ruber?7 and 8, the last of which seems to be one of the brightest metal-poor M?giants ever identified.
机译:目的借助可用的虚拟天文台工具,我们寻找了太阳附近的新M矮星和切向速度高的M巨人。方法。从光学Tycho-2和近红外2MASS目录之间的全天候交叉匹配中,我们选择了具有适当运动μ??> ?? 50?mas?yr-1和非常红色的VT ??? Ks颜色的对象。 。对于最有趣的目标,我们收集了多波长光度法,构建了光谱能量分布,通过对大气模型的拟合估算了有效温度和表面重力,对ASAS V波段光曲线进行了时间序列分析,并从低光谱中分配了光谱类型。 CAFOS在2.2?m的Calar Alto望远镜上获得的高分辨率光谱。结果。我们获得了59个明亮的红色高准运动物体的样本,其中包括五十个红色巨人,四个红矮星和五个在此工作中首次报告的物体。这五颗新星的星速为VT ??≈10.8-11.3?mag,减少了已知矮星与巨人之间的适当运动,巨人典型的近红外颜色,以及有效温度Teff ??≈2900-3400?K 。从时间序列分析中,我们发现在Ruber?4中有一个较长的中学期,在Ruber?6中发现了一个极长的初学者期。利用CAFOS光谱,我们确认了Ruber?7和Ruber 8的红色巨型性质,最后一个似乎是有史以来发现的最亮的金属贫乏的巨型巨人之一。

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